Apollo 12 Mission

Mission Photography

Apollo 12 represented man's second opportunity to directly observe scientific phenomena on
the lunar surface. Both the surface and orbital photography of the mission served not only to
document man's second lunar landing and extravehicular activities of the astronauts, but also
to identify scientifc areas and experiments for study in future missions. The photographic
equipment and materials carried by Apollo 12 were designed specifically to (1) photograph
targets of opportunity, i.e. scientifically interesting sites and potential Apollo landing
sites as time and circumstances permitted; (2) obtain photographs of the lunar module and lunar
surface activities after LM landing; (3) obtain multispectral, vertical, and oblique stereo
strips of nearside and farside regions of scientific interest; (4) record mission operational
activities; (5) obtain documentation for subsequent landing crew training purposes; and (6)
obtain photographic information to document the geologic samples.

70-millimeter Hasselblad EL Camera. This camera, which was carried aboard the
command module, featured a motor-drive mechanism, powered by two nickel-cadmium batteries that
advanced the film and cocked the shutter whenever the camera was activated.

70-millimeter Hasselblad Data Cameras. The two electrically powered data
cameras that were carried on the lunar module featured semiautomatic operation. They used a
60-millimeter Biogon lens exclusively. The operating sequence was initiated by squeezing a
trigger mounted on the camera handle. A 1-centimeter reseau grid was set in front of the
image plane to provide photogrammetric information in the analysis of the photography. The
cameras were bracket-mounted on the front of the LM astronauts' EVA suits.

16-millimeter Maurer Data Acquisition Camera. Apollo 12 carried two Maurer
data acquisition cameras (DAC), one in the command module and one in the lunar module. The
cameras were used primarily to record engineering data and for continuous-sequence terrain
photography. The CM camera had lenses of 50-, 10-, 18-, and 75-millimeter focal lengths; the
LM camera was fitted with a 10-millimeter wide-angle lens. Accessories included a right-angled
mirror, a power cable, a sextant adapter, a right-angled adapter, and a CM boresight window
bracket.

The Maurer cameras weighed 2.8 pounds each, with a 130-foot film magazine attached. They had
frame rates of 1, 6, and 12 fps automatic and 24 fps semiautomatic at all lens focal lengths,
and shutter speeds of 1/60, 1/125, 1/250, 1/500, and 1/1000 second, also at all lens focal
lengths.

35-mm Lunar Surface Close-up Stereoscopic Camera. This camera, which was carried on the lunar module's Modular Equipment Storage Assembly (MESA),
was designed for the highest possible resolution for a stereo pair area with a flash illumination
and fixed distance. Photography was accomplished by holding the camera on a walking stick
against the object to be photographed. The camera was powered by four nickel-cadmium batteries
that operated the motor drive mechanism and an electronic flash strobe light.

Four-Camera, Lunar Multispectral S-158 Experiment. The lunar multispectral camera (LMC) experiment used four Hasselblad EL cameras. The objectives
of the experiment were (1) to photograph lunar surface color variations for geologic mapping, (2)
to correlate photographs with spectral reflectance of returned samples for compositon
determination, (3) to photograph potential lunar landing sties, and (4) to make comparative
studies of lunar reflectance variation and wavelengths. (A similar experiment was flown as the
SO-65 Earth multispectral photography experiment on Apollo 9.)

The four cameras used had the same parameters, settings, and ranges as the Hasselblad EL
camera with the 80-millimeter lens. The cameras were mounted in a ring bracket perpendicular to
the command module hatch window ±5° from nadir, 57.5° pitched up from the X axis.
The shutters were automatically tripped by an intervalometer at 20-second intervals to obtain
vertical strip photography.

Orbital Photography

An important photographic objective was to obtain, from lunar orbit, photographs of future
landing sites. Orbital photographs did aid in the planning of pinpoint landings in lunar terrain
more rugged and of even greater scientific interest than the mare-type terrain at the Apollo 11 and 12 landing sites. Extensive landmark tracking and photography were performed in lunar orbit.
The lunar orbit photogrpahy was conducted using a 500-millimeter long-range lens to obtain
mapping and training data for future missions.

A high-oblique view looking northeast. This photograph was taken from the LM. The large
Copernicus Crater is in full view, and the Carpathian Mountain Range is visible on the horizon.
The stark lunar relief is accented by the low elevation angle of the Sun.

An oblique view looking northwest at the highland area north of Fra Mauro Crater. This
photograph was taken from the M at an orbital altitude of 60 nautical miles. The Sun was only
slightly higher when Apollo 13 landed in this area. (Arrow indicates landing site.)

Alphonsus, the target point of Ranger 9. The dark "haloed" areas on the floor of Alphonsus
are distinctly evident.These areas are of great geologic interest.

The difference between day and night on the Moon. The terminator is just to the west of
Gambart Crater, which is at the extreme north in the photograph. This view is representative
of the lunar surface as seen by the crew as they crossed the terminator twice every orbit. The Apollo 13 landing site is located in the highland region in the shadow area of the photograph.

Lunar Surface Photography

Following touchdown, photographs of the immediate vicinity of the Lunar Module were taken
through the LM windows. Shortly after both astronauts egressed the LM, the television camera
was inadvertently pointed directly at the Sun, and television coverage of the mission was lost.
Thus, the photographs taken by the crew are the only visual record of their
(1) surface activities,
(2) sample documentation, and
(3) stereoscopic surface photography.
Both crewmen took hundreds of photographs while on the surface.

Surface Activities. The lunar terrain over which the lunar module traveled during descent was documented by the
16-mm sequence camera. The 70-mm film exposed on the surface, when not affected by sun glint on
the lens or surface washout by sunlight, was generally of good quality.

Crew activities and lunar surface features near the lunar module, the experiment package, and
those observed during the two extravehicular excursions were well documented by still-camera
short sequences and by a number of panoramic views.

This mound on the lunar surface was photographed looking toward the southwest. This type of
feature and its formation have generated considerable interest among lunar geologists.

A close-up of the lower part of Surveyor 3. Those parts that were not returned to Earth were photographed extensively by the Apollo 12 crew.

Surveyor 3 with the LM in the background. Footpad 1 is to the left, footpad 2 is in the foreground, and the surface sampler extends to the right.

Astronaut Alan L. Bean, lunar module pilot for the Apollo 12 lunar landing mission, works at the Modular Equipment Stowage Assembly (MESA) on the Apollo 12 Lunar Module during the mission's first extravehicular activity, EVA 1, on November 19, 1969.

Sample Documentation. In addition to collecting samples, one of the main scientific tasks to be accomplished during
the extravehicular activities was photographing rocks, the lunar surface and the moonscape.

Sample 12052 before collection. The rock apparently was moved from the original site before the
photographs were taken. A drag mark near the sample indicates the place from which the rock was removed.

Sample 12052, a large rock rounded on one side, was collected from the west rim of Head Crater. Sample 12052 is shown as it was photographed on the lunar surface and as it was photoraphed in the Lunar Receiving Laboratory.

The third image is a photomicrograph of sample 12052.

Stereoscopic Closeup Surface.To obtain information about in-place lunar rocks and soil, a close-up stereoscopic camera
capable of photographing small-scale surface features was used at the Apollo 12 landing site.
The camera was the same type as the one used during the Apollo 11 mission. Fifteen stereoscopic
photograph pairs were obtained. The types of lunar surfaces photographed were (1) solid and
rock surfaces not greatly disturbed by the LM descent engine exhaust, (2) soil surfaces
disturbed by the LM descent engine exhaust, and (3) soil surfaces disturbed by astronaut
boots.

The rough, irregular soil surface has abundant 1- to 10- millimeter-long angular rock fragments embedded in the soil and lying loose on the surface. The composition of the fine-grained soil (grain size less than 1 millimeter) cannot be determined from the photograph. The particles with bright reflection in the photograph have the same general appearance as the brown glass droplets and angular fragments in the lunar soil samples. Glass is probably a significant component of the soil shown in the photograph.

The soil surface appears to be undisturbed by the LM descent engine exhaust. Clumps of soil and perhaps some soil-covered rock fragments are covered by a thin, irregular, moderately coherent crust, which was possibly cracked (cracks visible at the top of the photograph) by the downward pressure of the camera body on the soil. Nearly all loose surface fragments have either been incorporated into the crust or blown off. Rock fragments are difficult to identify in the photograph.

The soil surface has been swept by the LM descent engine exhaust, which left lineations.Depressions are left where 2- to 3- millimeter-diameter particles were possibly plucked out of the surface and swept along by the exhaust gases. The 1- to 10-millimeter-diameter particles lying loose on the surface appear to be mostly subrounded breccias, some with glass coatings.

The soil in the upper quarter of the area photographed was cohesive enough to form a vertical
wall at the edge of the exhaust-gas disturbance and for a clump of it to slide over the surface
without fragmenting (right center portion of the photograph). The photograph was possibly taken
of an area in which the soil had been compressed by the LM footpad.

Summary

The scientific, geologic, and photographic objectives of the Apollo 12 mission were designed to achieve the maximum return of lunar data. The staytime on the lunar surface was increased to accommodate two extravehicular activity periods. The photography accomplished during the Apollo 12 mission documented and augmented the experimental, observational, and geologic data obtained from the extended lunar surface activities and from the scientific instruments placed on the lunar surface. A further photographic objective was to obtain, from lunar orbit, photographs of future landing sites.

During the mission, all but two of 25 70-millimeter and 16-millimeter film magazines carried on board were returned exposed. A partially exposed 70-millimeter magazine had jammed and was inadvertently left on the lunar surface, and one 16-millimeter magazine was not used. Approximately 53% of the suggested targets of opportunity from lunar orbit were photographed.